If the Moon is brought closer to the Earth such that its distance from the Earth becomes half of the original distance, then the gravitational force of attraction between the Earth and the Moon would :
- (a)reduce to half of its original value
- (b)increase to two times of its original value
- (c)remain the same as the original value
- (d)increase to four times of its original value
Correct — D, increase to four times of its original value. Newton's law of universal gravitation says the pull between two bodies is F = GMm/r², where r is the distance between their centres. Neither mass changes here, so G, M and m stay put and the whole answer sits in the r² underneath. Replace r by r/2 and the denominator becomes (r/2)² = r²/4, which is a quarter of what it was; dividing by a quarter is multiplying by four. The force therefore rises to four times its original value. The general habit is worth fixing: because the distance is squared, a change in separation always bites twice as hard as the same change in a mass. Double the distance and the force falls to a quarter; treble it and the force falls to a ninth.
- (a)reduce to half of its original value — Gets both the direction and the size wrong. Bringing the bodies closer strengthens the attraction, and even the strengthening would not be a simple factor of two because the distance is squared.
- (b)increase to two times of its original value — The right direction with the wrong exponent. Doubling would be the answer if the force went as 1/r; it goes as 1/r², so the factor is 2² = 4.
- (c)remain the same as the original value — Would be true only if the force did not depend on separation at all. It does — distance is the one thing this question changes, and the force follows it.
Newton's law of universal gravitation states that every particle of matter attracts every other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them: F = GMm/r². The constant G is about 6·67 × 10⁻¹¹ N m² kg⁻², the same everywhere in the universe, and it is what makes gravitation utterly negligible between everyday objects and dominant between astronomical ones. The force is always attractive, acts along the line joining the two bodies, and forms an action–reaction pair — the Moon pulls on the Earth exactly as hard as the Earth pulls on the Moon.
This is a one-line inverse-square drill dressed up as an astronomy question, and the mention of the Moon is decoration. The safe method is to write the ratio rather than the formula: F_new/F_old = (r_old/r_new)², so halving the separation gives a ratio of 2² = 4. Doing it this way stops the two standard slips — forgetting to square, and getting the direction backwards. Note that the physical scenario is impossible in a stable sense: at half its distance the Moon would be inside the Roche limit region for tidal stress and the tides on Earth would be enormously stronger, since tidal effect falls off even faster, as 1/r³. The question asks only about the force between them, so none of that is needed for the mark, but it is why the item cannot be reasoned from intuition about orbits.
- The gravitational force between two bodies is F = GMm/r², with r measured centre to centre.
- The universal gravitational constant G is about 6·67 × 10⁻¹¹ N m² kg⁻² and does not change with place, medium or time.
- Halving the separation multiplies the force by four; doubling it divides the force by four.
- Gravitational force is always attractive and always acts along the line joining the two bodies, as an equal and opposite pair.
- The mean Earth–Moon distance is about 384,400 km, and the same inverse-square law is what holds the Moon in orbit and what raises the ocean tides.
- Forgetting to square the distance factor, which turns a factor of four into a factor of two.
- Reversing the direction — closer means a stronger pull, not a weaker one.
- Applying the same reasoning to tides, which weaken as the cube of the distance rather than the square.
Almost always as a proportional-change one-liner: change a mass, or the separation, or both, and state what happens to the force.
Two bodies of mass M each are placed R distance apart. In another system, two bodies of mass 2M are placed R/2 distance apart. If F be the gravitational force between the bodies in the first system, then the gravitational force between the bodies in the second system will be
- (a) 16 F
- (b) 1 F
- (c) 4 F
- (d) None of the above
Answer(a) 16 F
The fullest version of the same drill. Both masses double, giving four, and the separation halves, giving another four — sixteen in all, of which this question uses only the distance half.
CDS_GK_2020_II_Q872020If the distance between two objects is increased by two times, the gravitational force between them will
- (a) remain same
- (b) increase by two times
- (c) decrease by two times
- (d) decrease by four times
Answer(d) decrease by four times
The same inverse-square step, run the other way. There the separation doubles and the pull drops to a quarter; here it halves and the pull quadruples. Both hinge on the square in the denominator.
CDS_GK_2022_I_Q62022What happens to the gravitational force between two objects if the mass of one object is doubled and the distance between them is also doubled?
- (a) The force would remain the same
- (b) The force would be doubled
- (c) The force would be halved
- (d) The force would increase by a factor of 4
Answer(c) The force would be halved
A harder cousin, with a mass and the distance changing at once — the mass factor of two fights the distance factor of four and loses, so the force is halved.
- practice — not a real PYQ
If the masses of two bodies are each doubled and the distance between them is also doubled, the gravitational force between them will
- (a)remain the same
- (b)become half
- (c)become four times
- (d)become sixteen times
Answer(a) remain the same — the product of the masses goes up by four and the square of the distance also goes up by four, so the two changes cancel exactly.
- practice — not a real PYQ
The value of the universal gravitational constant G
- (a)is greater at the poles than at the equator
- (b)decreases with height above the Earth's surface
- (c)is the same everywhere in the universe
- (d)depends on the medium between the two bodies
Answer(c) is the same everywhere in the universe — G is a universal constant. It is g, the acceleration due to gravity, that varies with latitude, altitude and depth.